By using the identification scheme described in the previous section, we successfully identified 58 BVFs in the FUGIN \({\rm ^{12}CO}\)  J=1–0 data. Note that some previously known broad CO line features, such as the W44 “Bullet” ([1]}) or the shocked clumps in SNRs (e.g.,[2]}; [3]}), have not been identified in the current survey. This is due to the fact that \({\rm ^{12}CO}\)  J=1–0 emission from these features is weaker than the rms noise of the FUGIN data (\(\sim \!\!1.47 \rm \ K\) ; §2.1). A catalog of 58 BVFs is presented in Table REF  , and their images are shown in Appendix A.  Each BVF in the catalog is listed with the following set of parameters: the \((l, b)\)  location of the emission peak, velocity of the “parent" molecular cloud, sizes along the \(l\)  and \(b\)  axes (\(\Delta l\)  and \(\Delta b\) ), velocity width (\(\Delta V\) ), peak temperature, and \(^{13}\) CO/\(^{12}\) CO intensity ratio. The sizes and velocity width are defined by FWZI.
